The monopole and quadrupole moments of the epoch of reionization (EoR) 21-cm bispectrum

Author:

Gill Sukhdeep Singh1ORCID,Pramanick Suman1ORCID,Bharadwaj Somnath1,Shaw Abinash Kumar2ORCID,Majumdar Suman34ORCID

Affiliation:

1. Department of Physics, Indian Institute of Technology Kharagpur , Kharagpur 721302 , India

2. Astrophysics Research Center of the Open University (ARCO), The Open University of Israel , 1 University Road, Ra’anana 4353701 , Israel

3. Department of Astronomy, Astrophysics and Space Engineering, Indian Institute of Technology , Indore 453552 , India

4. Department of Physics, Blackett Laboratory, Imperial College , London SW7 2AZ , UK

Abstract

ABSTRACT We study the monopole ($\bar{B}^0_0$) and quadrupole ($\bar{B}^0_2$) moments of the 21-cm bispectrum (BS) from EoR simulations and present results for squeezed and stretched triangles. Both $\bar{B}^0_0$ and $\bar{B}^0_2$ are positive at the early stage of EoR where the mean neutral hydrogen (${\rm H\, {\small I}}$) density fraction $\bar{x}_{\rm {\rm H\, {\small I}}}\approx 0.99$. The subsequent evolution of $\bar{B}^0_0$ and $\bar{B}^0_2$ at large and intermediate scales (k = 0.29 and $0.56 \, {\rm Mpc}^{-1}$, respectively) is punctuated by two sign changes which mark transitions in the ${\rm H\, {\small I}}$ distribution. The first sign flip where $\bar{B}^0_0$ becomes negative occurs in the intermediate stages of EoR $(\bar{x}_{\rm {\rm H\, {\small I}}}\gt 0.5)$, at large scale first followed by the intermediate scale. This marks the emergence of distinct ionized bubbles in the neutral background. $\bar{B}^0_2$ is relatively less affected by this transition, and it mostly remains positive even when $\bar{B}^0_0$ becomes negative. The second sign flip, which affects both $\bar{B}^0_0$ and $\bar{B}^0_2$, occurs at the late stage of EoR $(\bar{x}_{\rm {\rm H\, {\small I}}}\lt 0.5)$. This marks a transition in the topology of the ${\rm H\, {\small I}}$ distribution, after which we have distinct ${\rm H\, {\small I}}$ islands in an ionized background. This causes $\bar{B}^0_0$ to become positive. The negative $\bar{B}^0_2$ is a definite indication that the ${\rm H\, {\small I}}$ islands survive only in underdense regions.

Funder

Israel Science Foundation

Science and Engineering Research Board

Department of Science and Technology

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 1 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Impact of astrophysical scatter on the epoch of reionization [H i]21 bispectrum;Journal of Cosmology and Astroparticle Physics;2024-08-01

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